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Diffraction - Astronomy Scientific Imaging Solutions Diffraction Limited’s line of high performance or “scientific grade” CCD and CMOS cameras are designed to operate under extremely low-light conditions with high sensitivity, low
MaxIm DL™ - Astronomy Scientific Imaging Solutions Registered users can optionally purchase a USB stick; please contact Diffraction Limited for more information Software Returns Policy All software sales are final A free demo period of the MaxIm DL Pro level software, with full technical support is available to determine suitability of the software prior to sale
Support - Astronomy Scientific Imaging Solutions - Diffraction Limited Factory Repairs Repairs for Aluma CCD, Aluma AC, StarChaser, and STC series cameras and accessories must be performed at the factory If you require service, please post in the Technical Support forum If a return is necessary then you will be issued an RMA number and shipping instructions
Cloud Sensor - Diffraction Limited The primary sensors used for determining safe unsafe observing conditions are cloud detection, rain detection, wind speed limits, and daylight The user can also set limits on other parameters, including humidity, temperature, etc
SBIG Aluma AC4040 - Diffraction Limited CMOS sensors often have more limited well depth and bit depth than their CCD predecessors At the same time, the modern CMOS sensors have much lower read noise than the equivalent CCD This low read noise can be used to advantage, by stacking many shorter exposures to achieve the same final result
Optical Aberrations - Diffraction Limited This is the so-called 1 4-wave " diffraction limit A term describing an optical system which is better than 1 4-wave accuracy peak-to-valley If an optical system is any worse than this, there is significant blurring of the image